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Hubble Tension Explanation from This Cosmological Model AΛΩ (Slow Bang Model, SB)
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作者 Jean Perron 《Journal of High Energy Physics, Gravitation and Cosmology》 CAS 2024年第1期106-125,共20页
In this article we present a model of Hubble-Lemaître law using the notions of a transmitter (galaxy) and a receiver (MW) coupled to a model of the universe (Slow Bang Model, SB), based on a quantum approach of t... In this article we present a model of Hubble-Lemaître law using the notions of a transmitter (galaxy) and a receiver (MW) coupled to a model of the universe (Slow Bang Model, SB), based on a quantum approach of the evolution of space-time as well as an equation of state that retains all the infinitesimal terms. We find an explanation of the Hubble tension H<sub>0</sub>. Indeed, we have seen that this constant depends on the transceiver pair which can vary from the lowest observable value, from photons of the CMB (theoretical [km/s/Mpc]) to increasingly higher values depending on the earlier origin of the formation of the observed galaxy or cluster (ETG ~0.3 [Gy], ~74 [km/s/Mpc]). We have produced a theoretical table of the values of the constant according to the possible pairs of transmitter/receiver in the case where these galaxies follow the Hubble flow without large disturbance. The calculated theoretical values of the constant are in the order of magnitude of all values mentioned in past studies. Subsequently, we applied the models to 9 galaxies and COMA cluster and found that the models predict acceptable values of their distances and Hubble constant since these galaxies mainly follow the Hubble flow rather than the effects of a galaxy cluster or a group of clusters. In conclusion, we affirm that this Hubble tension does not really exist and it is rather the understanding of the meaning of this constant that is questioned. 展开更多
关键词 Model of the Universe Cosmological Constant hubble Constant hubble’s Tension hubble-Lemaître Law hubble’s Flow
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Cosmological Implications of Diffusion: The Hubble Tension
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作者 Sebastiano Tosto 《Journal of Applied Mathematics and Physics》 2024年第12期4077-4097,共21页
The paper introduces an “ab initio” model to calculate the timeline of the temperature field of the Big Bang radiation field in the universe and its connection with the Hubble law. The theoretical approach is rooted... The paper introduces an “ab initio” model to calculate the timeline of the temperature field of the Big Bang radiation field in the universe and its connection with the Hubble law. The theoretical approach is rooted in the concept of quantum uncertainty and has a quantum character. The aim is to emphasize that the big bang energy diffusion throughout the expanding universe is enough to account also for the Hubble tension. 展开更多
关键词 Quantum Theory RELATIVITY Universe Timeline Universe Age hubble Tension
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The Hawking Hubble Temperature as the Minimum Temperature, the Planck Temperature as the Maximum Temperature, and the CMB Temperature as Their Geometric Mean Temperature
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作者 Espen Gaarder Haug Eugene Terry Tatum 《Journal of Applied Mathematics and Physics》 2024年第10期3328-3348,共21页
Using a rigorous mathematical approach, we demonstrate how the Cosmic Microwave Background (CMB) temperature could simply be a form of geometric mean temperature between the minimum time-dependent Hawking Hubble tempe... Using a rigorous mathematical approach, we demonstrate how the Cosmic Microwave Background (CMB) temperature could simply be a form of geometric mean temperature between the minimum time-dependent Hawking Hubble temperature and the maximum Planck temperature of the expanding universe over the course of cosmic time. This mathematical discovery suggests a re-consideration of Rh=ctcosmological models, including black hole cosmological models, even if it possibly could also be consistent with the Λ-CDM model. Most importantly, this paper contributes to the growing literature in the past year asserting a tightly constrained mathematical relationship between the CMB temperature, the Hubble constant, and other global parameters of the Hubble sphere. Our approach suggests a solid theoretical framework for predicting and understanding the CMB temperature rather than solely observing it.1. 展开更多
关键词 Hawking Temperature Planck Temperature CMB Temperature Geometric Mean Compton Wavelength hubble Sphere Cosmological Models
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Predicting High Precision Hubble Constant Determinations Based on a New Theoretical Relationship between CMB Temperature and H0
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作者 Eugene Terry Tatum Espen Gaarder Haug Stéphane Wojnow 《Journal of Modern Physics》 2024年第11期1708-1716,共9页
Based on considerable progress made in understanding the Cosmic Microwave Background (CMB) temperature from a deep theoretical perspective, this paper demonstrates a useful and simple relationship between the CMB temp... Based on considerable progress made in understanding the Cosmic Microwave Background (CMB) temperature from a deep theoretical perspective, this paper demonstrates a useful and simple relationship between the CMB temperature and the Hubble constant. This allows us to predict the Hubble constant with much higher precision than before by using the CMB temperature. This is of great importance, since it will lead to much higher precision in various global parameters of the cosmos, such as the Hubble radius and the age of the universe. We have improved uncertainty in the Hubble constant all the way down to 66.8712 ± 0.0019 km/s/Mpc based on data from one of the most recent CMB studies. Previous studies based on other methods have rarely reported an uncertainty much less than approximately ±1 km/s/Mpc for the Hubble constant. Our deeper understanding of the CMB and its relation to H0seems to be opening a new era of high-precision cosmology, which may well be the key to solving the Hubble tension, as alluded to herein. Naturally, our results should also be scrutinized by other researchers over time, but we believe that, even at this stage, this deeper understanding of the CMB deserves attention from the research community. 展开更多
关键词 hubble Constant CMB Planck Temperature Upsilon Constant
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How to Predict the Temperature of the CMB Directly Using the Hubble Parameter and the Planck Scale Using the Stefan-Boltzmann Law
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作者 Espen Gaarder Haug Stéphane Wojnow 《Journal of Applied Mathematics and Physics》 2024年第10期3552-3566,共15页
Based on recent progress in quantum gravity and quantum cosmology, we are also presenting a way to estimate the temperature in the cosmos, the Hubble sphere, from a relation between the Planck temperature and the Hubb... Based on recent progress in quantum gravity and quantum cosmology, we are also presenting a way to estimate the temperature in the cosmos, the Hubble sphere, from a relation between the Planck temperature and the Hubble scale. Our analysis predicts the Hubble sphere temperature of 2.72 K with the one standard deviation confidence interval between 2.65 K and 2.80 K, which corresponds well with the measured temperature observed from the cosmic microwave background (CMB) of about 2.72 K. This adds evidence that there is a close connection between the Planck scale, gravity, and the cosmological scales as anticipated by Eddington already in 1918.1. 展开更多
关键词 CMB Temperature hubble Parameter Stefan-Boltzmann Law Planck Scale
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A Comment on the Hubble Expansion Parameter Tension
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作者 Bruce Hoeneisen 《International Journal of Astronomy and Astrophysics》 2024年第1期61-64,共4页
We point out that the recent baryon acoustic oscillation measurement by the Dark Energy Survey collaboration relieves the Hubble expansion parameter tension.
关键词 hubble Parameter H0 Tension
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Hubble常数的Bayes估计
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作者 陈黎 王晓峰 李宗伟 《北京师范大学学报(自然科学版)》 CAS CSCD 北大核心 2000年第4期458-462,共5页
将 Bayes统计应用于 Hubble常数 H0 的 4类模型 :Ia型超新星、Tully- Fisher关系 ,星族 及 Sunyaev- Zel'dovich效应 .在 68.3%置信水平上得到的 H0 的 Bayes估计为 61.6<H0 <66.8( km· s-1· Mpc-1) ,由之导出的... 将 Bayes统计应用于 Hubble常数 H0 的 4类模型 :Ia型超新星、Tully- Fisher关系 ,星族 及 Sunyaev- Zel'dovich效应 .在 68.3%置信水平上得到的 H0 的 Bayes估计为 61.6<H0 <66.8( km· s-1· Mpc-1) ,由之导出的宇宙年龄约 ( 15± 1)× 10 9a,与利用球状星团测龄的结果 ( 15± 3)× 10 展开更多
关键词 宇宙学 hubble常数 Bayes统计方法
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Extended Hubble Diagram on the Basis of Gamma Ray Bursts Including the High Redshift Range of z = 0.0331 - 8.1 被引量:2
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作者 Laszlo A. Marosi 《International Journal of Astronomy and Astrophysics》 2019年第1期1-11,共11页
It is generally accepted that the history of the expansion of the universe can be exactly described by the concordance model, which makes specific predictions about the shape of the Hubble diagram. The redshift-magnit... It is generally accepted that the history of the expansion of the universe can be exactly described by the concordance model, which makes specific predictions about the shape of the Hubble diagram. The redshift-magnitude Hubble diagram in the redshift range z = 0.0104 - 1 seems to confirm this expectation, and it is believed that this conformity is also valid in the high redshift range. However, this belief is not undisputed. Recent work in the high redshift range of up to z = 8.1 has shown that the shape of the Hubble diagram deviates considerably from the predictions made by the Lambda cold dark matter model. These analyses, however, were based on mixed SN1a and gamma ray burst data, and some astronomers argue that this may have biased the results. In this paper, 109 cosmology-independent, calibrated gamma ray burst z/&mu;data points are used to calculate the Hubble diagram in the range z = 0.034 to z = 8.1. The outcome of this analysis confirms prior results: contrary to expectations, the shape of the Hubble diagram turns out to be exponential, and this is difficult to explain within the framework of the standard model. The cosmological implications of this unexpected result are discussed. 展开更多
关键词 REDSHIFT Gamma Ray BURSTS hubble DIAGRAM EXPONENTIAL Slope hubble’s Law ΛCDM Model
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Relativistic Quantitative Determination of the “Mysterious” Differences in the Hubble Constant 被引量:1
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作者 Ernst Karl Kunst 《Natural Science》 2021年第1期1-7,共7页
This paper discusses the “Hubble constant measurement—mystery”. Independent measurements of this cosmic parameter, referred to as <i><span style="font-family:Verdana;">H</span></i>... This paper discusses the “Hubble constant measurement—mystery”. Independent measurements of this cosmic parameter, referred to as <i><span style="font-family:Verdana;">H</span></i><sub><span style="font-family:Verdana;">0</span></sub><span style="font-family:Verdana;"> in abbreviated form, have all led to different values, with the highest value ≈ 74 km<span style="font-family:Verdana, Helvetica, Arial;white-space:normal;background-color:#FFFFFF;">·</span>s</span><sup><span style="font-family:Verdana;">-1</span></sup><span style="font-family:Verdana;"><span style="font-family:Verdana, Helvetica, Arial;white-space:normal;background-color:#FFFFFF;">·</span>Mpc</span><sup><span style="font-family:Verdana;">-1</span></sup><span style="font-family:Verdana;"> and the lowest ≈ 67 km<span style="font-family:Verdana, Helvetica, Arial;white-space:normal;background-color:#FFFFFF;">·</span>s</span><sup><span style="font-family:Verdana;">-1</span></sup><span style="font-family:Verdana;"><span style="font-family:Verdana, Helvetica, Arial;white-space:normal;background-color:#FFFFFF;">·</span>Mpc</span><sup><span style="font-family:Verdana;">-1</span></sup><span style="font-family:Verdana;">, where km denotes kilometer, s second and Mpc</span><sup><span style="font-family:Verdana;">-1</span></sup><span style="font-family:Verdana;"> megaparsec. These measurements have mainly been obtained with space telescopes. Apparently, up to now there was no way to explain the differences. However, previously published studies seem to regard the problem of the different measurement results for </span><i><span style="font-family:Verdana;">H</span></i><sub><span style="font-family:Verdana;">0</span></sub><span style="font-family:Verdana;"> [</span><span style="font-family:Verdana;"><a href="#ref1">1</a>,</span><b><span style="font-family:Verdana;"> </span></b><span style="font-family:Verdana;"><a href="#ref2">2</a></span><span style="font-family:Verdana;">]. I have shown that due to a symmetrical expansion of the Minkowski space (SMS), each respective frame of reference for an observer, who rests in the zero point of the frame, is converted into a state of apparent rest relative to the cosmic microwave background (CMB) radiation. This SMS-relativistic effect also seems to be responsible for the different measurement results of the Hubble constant, especially through space telescopes.</span> 展开更多
关键词 hubble Constant Different Measurement Results Earthbound and Space-Telescopes Different Orbits Different hubble Constants Symmetric Special Relativistic Origin
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旋涡星系随Hubble序列的一些统计性质 被引量:3
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作者 马骏 赵君亮 +1 位作者 张飞鹏 彭秋和 《天文学报》 CSCD 北大核心 2000年第2期172-180,共9页
对发表在A&ApSupplementSeries上的 365个旋涡星系的一些参数 (如表示旋臂缠卷松紧程度的参数Λ、切向角 μ、盘的扁度H/D2 5以及厚度等 )随Hubble序列变化的关系进行了统计研究 .首次得到这些参量的平均值 ;并且从统计结果可以明... 对发表在A&ApSupplementSeries上的 365个旋涡星系的一些参数 (如表示旋臂缠卷松紧程度的参数Λ、切向角 μ、盘的扁度H/D2 5以及厚度等 )随Hubble序列变化的关系进行了统计研究 .首次得到这些参量的平均值 ;并且从统计结果可以明显地看到Hubble对旋涡星系的分类只是一种定性的、只有统计意义上的分类 ;另外 ,从我们的统计结果看 ,密度波理论的色散关系对大多数旋涡星系是成立的 。 展开更多
关键词 旋涡星系 旋臂 切向角 统计关系 hubble序列
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The Hubble Field vs Dark Energy
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作者 Juan Lartigue 《Journal of Modern Physics》 2016年第12期1607-1615,共9页
The Hubble equation was considered valid enough to calculate the recession velocity of galaxies, until further observations showed that there would be an accelerated recession in the Hubble flow, necessarily tied to a... The Hubble equation was considered valid enough to calculate the recession velocity of galaxies, until further observations showed that there would be an accelerated recession in the Hubble flow, necessarily tied to an accelerated expansion of the Universe. So, this paper postulates the existence of a Hubble field as a possible cause for such an accelerated expansion, with some conditions: it must be a scalar field whose intensity should be a constant in respect to distance and whose Poisson equation should not be zero nor a function of mass;such field could rather be a property of the space-time. The obvious expression for acceleration should be the derivative of the Hubble equation respect to time, which gives two opposed-signs terms whose substitution by the De-Sitter equation drives to a permanent negative acceleration, similarly to that obtained by the 2<sup>nd</sup> Friedmann equation. Otherwise, the inclusion of the ? term in the gravitational Einstein equation has led to a two opposed-signs terms expression, resembled to a non-published Newton equation. The negative term expresses the gravitational attraction and the positive one expresses the accelerated expansion as a ? function, which usually is attributed to dark energy. In this paper it is shown that Λ is proportional to the squared Hubble parameter and that the uncertain dark energy may be substituted by the calculable Hubble field intensity to obtain an equation for the net Universe acceleration. Equations for the Hubble parameter as functions of time and radius are also deduced. A relation is shown between the various assumed masses of the Universe and its critical radius. Additional Universe parameters are estimated such as the deceleration factor and a solution for the Poisson equation in the Hubble field. A brief comment t on high-standard candles is included. 展开更多
关键词 hubble Law hubble Field Cosmological Constant Friedmann Equations
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A New Physics Would Explain What Looks Like an Irreconcilable Tension between the Values of Hubble Constants and Allows <i>H<sub>0</sub></i>to Be Calculated Theoretically Several Ways
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作者 Claude Mercier 《Journal of Modern Physics》 2021年第12期1656-1707,共52页
<p> Observing galaxies receding from each other, Hubble found the universe’s expansion in 1929. His law that gives the receding speed as a function of distance implies a factor called Hubble constant <em>... <p> Observing galaxies receding from each other, Hubble found the universe’s expansion in 1929. His law that gives the receding speed as a function of distance implies a factor called Hubble constant <em>H</em><sub><em>0</em></sub>. We want to validate our theoretical value of <em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub> ≈ 72.09548580(32) km<span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span></span>s<span style="white-space:nowrap;"><span style="white-space:nowrap;"><sup><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></sup></span></span><sup>1</sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span></span>MParsec<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span></span>1</sup> with a new cosmological model found in 2019. This model predicts what may look like two possible values of <em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub>. According to this model, the correct equation of the apparent age of the universe gives ~ 14.14 billion years. In approximation, we get the well-known equation 1/<em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub> ≈ 13.56 billion years. When we force these ages to fit the 1/<em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub> formula, it gives two different Hubble constant values of ~69.2 and 72.1 km<span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span></span></span>s<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span></span>1</sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span><span style="white-space:nowrap;">sdot;</span></span></span></span></span>MParsec<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span></span>1</sup>. When we apply a theoretical correction factor of <em>η</em> ≈ 1.042516951 on the first value, both target the second one. We found 42 equations of <em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub> linking different physics constants. Some are used to measure <em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub> as a function of the average temperature<em> T</em> of the Cosmological Microwave Background and the universal gravitational constant <em>G</em>: </p> <p> <em>H</em><sub><em>0</em></sub> ≈ 72.06(90) km<span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span>s<span style="vertical-align:super;white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span><sup>1</sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span>MParsec<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span>1</sup> from <em>T </em>by Cobra probe & Equation (16) </p> <p> <em>H</em><sub><em>0</em></sub> ≈ 71.95(50) km<span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span>s<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span>1</sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span>MParsec<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span>1 </sup>from<em> T</em> by Partridge & Equation (16) </p> <p> <em>H</em><sub><em>0</em></sub> ≈ 72.086(36) km<span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span>s<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span>1</sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span>MParsec<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-1 </span></span></span></sup>from <em>G</em> & Equation (34) </p> <p> <em>H</em><sub><em>0</em></sub> ≈ 72.105(36) km<span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span>s<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span>1</sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span>MParsec<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span>1</sup> from <em></em><em>G</em> & Equations (74), (75), or (76). With 508 published values, <em>H</em><sub><em>0</em></sub> ≈ 72.0957 ± 0.33 km<span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span>s<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span>1</sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">&sdot;</span></span></span></span>MParsec<sup><span style="white-space:nowrap;"><span style="white-space:nowrap;"><span style="white-space:nowrap;">-</span></span></span>1</sup> seems to be the “ideal” statistical result. It validates our model and our theoretical <em>H</em><sub><em>0</em></sub> value which are useful to find various interactions with the different constants. Our model also explains the ambiguity between the different universe’s age measurements and seems to unlock a tension between two <em>H</em><sub><em>0</em></sub> values. </p> 展开更多
关键词 hubble Constant H0 hubble Tension Age of the Universe
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Hubble telescope 30 years in orbit:personal reflections 被引量:3
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作者 Robert Williams 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2020年第4期1-6,共6页
With an initial requirement to make observations a minimum of 5–10 years,Hubble Space Telescope(HST)has continued to operate well for 30 years.It has relied upon five servicing missions to repair and replace essentia... With an initial requirement to make observations a minimum of 5–10 years,Hubble Space Telescope(HST)has continued to operate well for 30 years.It has relied upon five servicing missions to repair and replace essential components.Since the final Space Shuttle mission 10 years ago,it has avoided major breaks in its operation,with the only serious effects of aging in space being a progressive deterioration in the performance of the gyroscopes and sensitivity of the instrument detectors.A number of factors were important in making HST a scientific landmark.Ground-breaking discoveries have been made with HST-the most important being the discovery of cosmic acceleration.When HST operation ceases,future observations in space should be assured with successful operation of major missions now planned by NASA,ESA,and the Chinese and Japanese Space Agencies. 展开更多
关键词 HST COSMIC acceleration hubble constant SUPERNOVAE
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基于Hubble.net的仓储系统设计与实现
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作者 杨伟超 马增军 耿卫 《计算机技术与发展》 2017年第10期181-184,188,共5页
科学技术的飞速发展,各类知识信息的爆发式增长,对高校的专业设置及其教学内容均带来了巨大的影响。图书馆作为学校文献资料的综合保障中心,面临着知识爆炸的严峻挑战。为此,借鉴当前最新的搜索引擎技术,设计并开发实现了基于Hubble.ne... 科学技术的飞速发展,各类知识信息的爆发式增长,对高校的专业设置及其教学内容均带来了巨大的影响。图书馆作为学校文献资料的综合保障中心,面临着知识爆炸的严峻挑战。为此,借鉴当前最新的搜索引擎技术,设计并开发实现了基于Hubble.net的仓储资源服务系统。该系统根据数字资源存储的特点,通过对图书馆资源进行对接整合并构建面向读者的数据库系统来存储和索引数据,同时内置了Web服务功能,以实现对图书馆内部电子信息与文献资料资源的充分利用。运行情况表明,所设计构建的仓储服务系统能够满足用户快速获取知识的需求,具有较强的稳定性和实用性,能够更加便捷有效地为图书馆用户提供高质量的服务。 展开更多
关键词 hubble.net 搜索引擎 仓储管理 海量数据
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搜索引擎Hubble.Net的机制分析及基础应用 被引量:1
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作者 赵英 《装备制造技术》 2011年第12期53-56,共4页
介绍了Hubble.Net的实现机制和对其结构进行了分析,对Hubble.Net的工具和类库作了讲解说明,并给出Hubble.Net在项目中的基础应用。
关键词 全文检索 hubble.Net 盘古分词
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Prospect for Cosmological Parameter Estimation Using Future Hubble Parameter Measurements 被引量:1
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作者 Jia-Jia Geng Rui-Yun Guo +2 位作者 An-Zhong Wang Jing-Fei Zhang Xin Zhang 《Communications in Theoretical Physics》 SCIE CAS CSCD 2018年第10期445-450,共6页
We constrain cosmological parameters using only Hubble parameter data and quantify the impact of future Hubble parameter measurements on parameter estimation for the most typical dark energy models. We first constrain... We constrain cosmological parameters using only Hubble parameter data and quantify the impact of future Hubble parameter measurements on parameter estimation for the most typical dark energy models. We first constrain cosmological parameters using 52 current Hubble parameter data including the Hubble constant measurement from the Hubble Space Telescope. Then we simulate the baryon acoustic oscillation signals from WFIRST(Wide-Field Infrared Survey Telescope) covering the redshift range of z ∈ [0.5, 2] and the redshift drift data from E-ELT(European Extremely Large Telescope) in the redshift range of z ∈ [2, 5]. It is shown that solely using the current Hubble parameter data could give fairly good constraints on cosmological parameters. Compared to the current Hubble parameter data, with the WFIRST observation the H(z) constraints on dark energy would be improved slightly, while with the E-ELT observation the H(z) constraints on dark energy is enormously improved. 展开更多
关键词 dark energy cosmological parameter constraints hubble parameter measurements
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Hubble Diagram Test of 280 Supernovae Redshift Data 被引量:2
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作者 Laszlo A. Marosi 《Journal of Modern Physics》 2014年第1期29-33,共5页
We compare the Hubble diagram calculated from the observed redshift (RS)/magnitude (μ) data of 280 Supernovae in the RS range of z = 0.0104 to 8.1 with Hubble diagrams inferred on the basis of the exponential tired l... We compare the Hubble diagram calculated from the observed redshift (RS)/magnitude (μ) data of 280 Supernovae in the RS range of z = 0.0104 to 8.1 with Hubble diagrams inferred on the basis of the exponential tired light and the Lambda Cold Dark Matter (ΛCDM) cosmological model. We show that the experimentally measured Hubble diagram follows clearly the exponential photon flight time (tS)/RS relation, whilst the data calculated on the basis of the ΛCDM model exhibit poor agreement with the observed data. 展开更多
关键词 Redshift/Magnitude DATA Fitting Linear hubble RELATION Exponential hubble RELATION ΛCDM COSMOLOGICAL Model
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Prediction and Derivation of the Hubble Constant from Subatomic Data Utilizing the Harmonic Neutron Hypothesis 被引量:2
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作者 Donald William Chakeres Richard Vento 《Journal of Modern Physics》 2015年第3期283-302,共20页
Purpose: To accurately derive H0 from subatomic constants in abscence of any standard astronomy data. Methods: Recent astronomical data have determined a value of Hubble’s constant to range from 76.9+3.9-3.4+10.0-8.0... Purpose: To accurately derive H0 from subatomic constants in abscence of any standard astronomy data. Methods: Recent astronomical data have determined a value of Hubble’s constant to range from 76.9+3.9-3.4+10.0-8.0 to 67.80 ± 0.77 (km/s)/Mpc. An innovative prediction of H0 is obtained from harmonic properties of the frequency equivalents of neutron, n0, in conjunction with the electron, e;the Bohr radius, α0;and the Rydberg constant, R. These represent integer natural unit sets. The neutron is converted from its frequency equivalent to a dimensionless constant,, where “h” = Planck’s constant, and “s” is measured in seconds. The fundamental frequency, Vf, is the first integer series set . All other atomic data are scaled to Vf as elements in a large, but a countable point set. The present value of H0 is derived and ΩM assumed to be 0. An accurate derivation of H0 is made using a unified power law. The integer set of the first twelve integers N12 {1,2,…,11,12}, and their harmonic fractions exponents of Vf represent the first generation of bosons and particles. Thepartial harmonic fraction, -3/4, is exponent of Vf which represents H0. The partial fraction 3/4 is associated with a component of neutron beta decay kinetic energy. Results: H0 is predicted utilizing a previously published line used to derive Planck time, tp. The power law line of the experimental H0 and tp conforms to the predicted line. Conclusions: H0 can be predicted from subatomic data related to the neutron and hydrogen. 展开更多
关键词 hubble Constant NEUTRON Unification Model PLANCK Time Quantum Gravity NEUTRON Beta Decay NEUTRINO
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基于Hubble.Net的加密文档检索系统
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作者 凌晔华 庞抗 +1 位作者 张晓洁 郑鑫 《智能计算机与应用》 2017年第3期79-81,共3页
针对当前企业对文档保密与检索功能的双重需求,提出一种添加模糊匹配Hubble.Net保密文档专用检索阅读方法。采用AES(Advanced Encryption Standard)加密算法对将加密文档提取的流信息流进行加密,使用Hubble.Net与对加密文档进行检索时,... 针对当前企业对文档保密与检索功能的双重需求,提出一种添加模糊匹配Hubble.Net保密文档专用检索阅读方法。采用AES(Advanced Encryption Standard)加密算法对将加密文档提取的流信息流进行加密,使用Hubble.Net与对加密文档进行检索时,而模糊匹配算法的使用大大增加了字符比对的容错性,在保证文档加密的同时兼顾了文档位置定位、关键字定位等文档检索功能。在检索速度及精度方面,要优于现有的方法。 展开更多
关键词 文档检索 hubble.Net 模糊匹配 AES加密
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Locally Varying Hubble Parameter in Terms of Reduced Friedmann Equation 被引量:1
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作者 Ayman Kassem 《International Journal of Astronomy and Astrophysics》 2021年第2期175-189,共15页
Assessment of the Hubble parameter as an indicator of the expansion rate of the universe holds a central position in the field of astronomy. From its initial estimate of about 500 km<span style="white-space:no... Assessment of the Hubble parameter as an indicator of the expansion rate of the universe holds a central position in the field of astronomy. From its initial estimate of about 500 km<span style="white-space:nowrap;">&sdot;</span>sec<sup>-1</sup><span style="white-space:nowrap;">&sdot;</span>parsc<sup>-1</sup>, this value had been steadily amended as the observational tools became more accurate and precise. Despite this, a gap remains between the value of observations relating to local and nonlocal estimations of the Hubble parameter that gave rise to what became known as the Hubble tension. This tension is addressed here while dealing with space fabric as a cosmological fluid that undergoes transition. 展开更多
关键词 Cosmic Fluid Transition Locally Varying hubble Parameter Energy Degrees of Freedom
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